Thermal Fluctuations and Black Hole Entropy
Gilad Gour, A.J.M. Medved

TL;DR
This paper investigates how thermal fluctuations influence black hole entropy, revealing that quantum corrections are logarithmic and depend on charge fluctuations, with implications for black hole thermodynamics in various models.
Contribution
It introduces a novel approach considering black hole quantum spectra and distinguishes between fixed and fluctuating charge systems using different statistical ensembles.
Findings
Quantum correction to entropy is logarithmic in classical entropy.
Charge fluctuations are significant even at zero net charge.
Asymptotically flat black holes cannot reach thermal equilibrium.
Abstract
In this paper, we consider the effect of thermal fluctuations on the entropy of both neutral and charged black holes. We emphasize the distinction between fixed and fluctuating charge systems; using a canonical ensemble to describe the former and a grand canonical ensemble to study the latter. Our novel approach is based on the philosophy that the black hole quantum spectrum is an essential component in any such calculation. For definiteness, we employ a uniformly spaced area spectrum, which has been advocated by Bekenstein and others in the literature. The generic results are applied to some specific models; in particular, various limiting cases of an (arbitrary-dimensional) AdS-Reissner-Nordstrom black hole. We find that the leading-order quantum correction to the entropy can consistently be expressed as the logarithm of the classical quantity. For a small AdS curvature parameter and…
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